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http://www.cosmosmagazine.com/node/3263/full
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David
Universe has less time left than thought
Friday, 29 January 2010
by Meghan Bergamin
Cosmos Online
SYDNEY: The amount of entropy, or disorder, in the observable universe is 30 times higher than previous estimates, report Australian astronomers, suggesting the universe may not have as much time left as previously thought.
Supermassive black holes, dark matter and stars are some of the contributors to the overall entropy of the universe, which is a measure of the irreversible processes occurring throughout.
Previous estimations of the total entropy of the universe were limited by insufficient measurements of supermassive black holes, as well as uncertainty about the entropy of dark matter, according to a study to be published in the Astrophysical Journal.
New advances on an old problem
The concept of entropy, which has existed in physics for almost 200 years, is central to the second law of thermodynamics and relates to the tendency of order in the universe to progressively turn to disorder.
Entropy is an important contributor to our understanding of both cosmology and biology. Life, along with every other chemical or physical process, cannot occur without producing entropy.
Everything from gravitational clustering, to supernovae, to the biological processes in our own bodies are contributors to the entropy budget of the universe; a budget which has been found to be 30 times larger than previously suspected, according to research by astrophysicists Chas Egan and Charles Lineweaver, from the Australian National University in Canberra.
“The work of Egan and Lineweaver is a significant advance in tallying the known sources of entropy in the universe,” says Adelaide based astrophysicist Roger Clay.
Gas tank of the universe running low
All particles in the universe emit energy as radiation, which results in entropy being produced. The amount of radiation emitted by a particle usually correlates to the temperature – high radiation produces high temperatures.
Entropy results from radiation as well as gravitation emissions, so calculating the amount of entropy in the entire observable universe involves identifying the major radiation and gravitation producing objects and their approximate number and size. Once this is known, entropy can be estimated by converting the known temperature of particles into units of energy.
Lineweaver describes the universe as a giant engine; the more efficient the engine, the lower the total entropy produced. His findings show that engine of our universe has a lot less gas left in the tank than we thought.
“It’s like driving along, thinking you have half a tank of gas, but when you get out and check it with a dipstick, you find you only have about a third of a tank.”
Supermassive black holes biggest entropy contributors
Using recent measurements of Stephen Hawking's supermassive black hole mass function, Egan and Lineweaver were able to produce a more accurate quantification of entropy.
Their calculations revealed that supermassive black holes, such as the one at the centre of the Milky Way, were the biggest contributors to the universe’s entropy in its entirety.
The approximate entropy of dark matter was also included for the first time. Dark matter emits no radiation, but can be detected by its gravitational effects on visible matter.
As it produces no radiation, dark matter does not produce a large amount of entropy when compared with visible matter, but it is still considered an important inclusion in the overall total, as there are large quantities of dark matter in the universe.
“In recent times, some of the most famous names in theoretical astrophysics and cosmology have been associated with trying to understand the entropy of the universe and its most esoteric members, the black holes and the dark matter,” says Clay.
Previous estimates of the amount of entropy in the observable universe place it at around 10102k - 10103kk represents the Boltzmann constant (a number which relates energy to temperature). Lineweaver says this is an underestimate by a factor of 30. joules per degree Celsius, where k represents the Boltzmann constant (a number which relates energy to temperature). Lineweaver says this is an underestimate by a factor of 30.
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